Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Exposure of South Polar Layered Deposits:   ESP_022839_0930   ESP_023009_0930   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.1

141.

0.01

14.35

71.4

71.9

Bedrock Exposed in 60-Kilometer Crater East of Valles Marineris:   ESP_023027_1740   ESP_029884_1740   (Interval in Earth days: 535)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.80

328.

7

22.75

33.0

50.6

Interior Layered Deposits on Floor of Depression:   ESP_022706_1485   ESP_022772_1485   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.1

95.4

8.63

-13.5

32.6

34.2

Proposed Landing Site in Ismenius Cavus:   ESP_022880_2140   ESP_031161_2140   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.82

17.2

-0.3

23.84

60.4

65.9

Layered Deposits and Possible MSL Rover Landing Site in Niesten Crater:   ESP_022892_1520   ESP_022470_1520   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

57.8

-3.8

11.01

32.8

33.0

Knob in South Polar Layered Deposits:   ESP_023066_0955   ESP_032020_0955   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.4

12.1

6.73

-6.06

70.6

73.7

Branching Trough in South Polar Layered Deposits:   ESP_022779_0950   ESP_031930_0950   (Interval in Earth days: 713)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.7

301.

-5.7

5.098

68.1

71.8

Remnant of Smooth Deposit:   ESP_022732_1375   ESP_023444_1375   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.9

107.

5.60

20.91

36.6

42.4

Multiple Eras of Gully Activity along Southern Hemisphere Crater Wall:   ESP_022841_1300   ESP_022986_1300   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.7

13.7

-5.1

5.814

42.1

42.7

Alluvial Fans and Inverted Channels in Kasimov Crater:   ESP_022829_1550   ESP_030609_1550   (Interval in Earth days: 606)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.6

337.

-6.8

8.908

32.6

40.6


  


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